Circumstellar Origin of Chrysene (C <sub>18</sub> H <sub>12</sub> ) via Self‐Recombination of Resonantly‐Stabilized 1‐Indenyl Radicals and Implications to the Aromaticity of the Carbonaceous Asteroid Ryugu

) in an overall endoergic reaction. These features account for the circumstellar origin of chrysene in pristine samples of the carbonaceous asteroid Ryugu and of the Murchison meteorite. At the microscopic level, the ring expansion involving cyclopentadienyl moieties to two six-membered aromatic rings via pivotal spiroaromatic intermediates affords a versatile, RSFR-initiated mass growth channel essentially leading to graphene-type PAHs and eventually two-dimensional nanostructures in high temperature circumstellar envelopes and in combustion processes.

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Publication Details

Journal
Angewandte Chemie International Edition
Published
2026-04-30
DOI
https://doi.org/10.1002/anie.8986387
Primary Topic
Astro and Planetary Science
Type
article
Field-Weighted Citation Impact
0.00

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article

Circumstellar Origin of Chrysene (C 18 H 12 ) via Self‐Recombination of Resonantly‐Stabilized 1‐Indenyl Radicals and Implications to the Aromaticity of the Carbonaceous Asteroid Ryugu

Valeriy N. Azyazov, Vladislav S. Krasnoukhov, Souvick Biswas, Shane J. Goettl et al.
Angewandte Chemie International Edition
Astro and Planetary Science
article

Circumstellar Origin of Chrysene (C 18 H 12 ) via Self‐Recombination of Resonantly‐Stabilized 1‐Indenyl Radicals and Implications to the Aromaticity of the Carbonaceous Asteroid Ryugu

Valeriy N. Azyazov, Vladislav S. Krasnoukhov, Souvick Biswas, Shane J. Goettl, Musahid Ahmed, Alexander Moiseevich Mebel, Nureshan Dias, Stanislaw F Wnuk, Sabrina Arias, Ralf I Kaiser
article en

Abstract

) in an overall endoergic reaction. These features account for the circumstellar origin of chrysene in pristine samples of the carbonaceous asteroid Ryugu and of the Murchison meteorite. At the microscopic level, the ring expansion involving cyclopentadienyl moieties to two six-membered aromatic rings via pivotal spiroaromatic intermediates affords a versatile, RSFR-initiated mass growth channel essentially leading to graphene-type PAHs and eventually two-dimensional nanostructures in high temperature circumstellar envelopes and in combustion processes.

Angewandte Chemie International Edition
University of Hawaiʻi at Mānoa (US), Lawrence Berkeley National Laboratory (US), Florida International University (US), Samara National Research University (RU)
Basic Energy Sciences
Openalex Percentile: Top 12%
Astro and Planetary Science
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